Finally, we recall that the results obtained in this paper refer to the AGN effect on the morphological properties of their host galaxies at z \(\sim \)  0. When going to higher redshifts and fainter magnitudes, and due to the effect that both the survey depth and resolution have on the morphological classification of galaxies, the study will be more complex, as mentioned above and analysed in detail in [1]}. We plan to proceed with this approach in a forthcoming paper (Getachew et al., in prep.).
